MARC보기
LDR02283nam u200433 4500
001000000421476
00520190215165339
008181129s2018 |||||||||||||||||c||eng d
020 ▼a 9780438382176
035 ▼a (MiAaPQ)AAI10815303
035 ▼a (MiAaPQ)colorado:15539
040 ▼a MiAaPQ ▼c MiAaPQ ▼d 247004
0820 ▼a 523
1001 ▼a Zetterlund, Erika. ▼0 (orcid)0000-0001-7007-6850.
24510 ▼a Fuel for the Star Formation Engine: Dense Molecular Cloud Clumps in the Northern Galactic Plane.
260 ▼a [S.l.]: ▼b University of Colorado at Boulder., ▼c 2018.
260 1 ▼a Ann Arbor: ▼b ProQuest Dissertations & Theses, ▼c 2018.
300 ▼a 204 p.
500 ▼a Source: Dissertation Abstracts International, Volume: 80-02(E), Section: B.
500 ▼a Adviser: Jason Glenn.
5021 ▼a Thesis (Ph.D.)--University of Colorado at Boulder, 2018.
520 ▼a The interstellar medium (ISM) is a confusing, muddled place. It provides the fuel for star formation, but before that can occur, the ISM must cool and condense into molecular clouds. Even this is not enough, however. It is only the cores, contai
520 ▼a I use the Herschel infrared GALactic plane survey (Hi-GAL) to study molecular cloud clumps through their thermal dust emission at 500 microm. For adapting and testing the clump identification and distance techniques---developed for the Bolocam G
520 ▼a The application of these techniques to 10° < &ell
520 ▼a Finally, with the addition of a catalog of clouds produced using the CO High Resolution Survey (COHRS), I addressed molecular cloud clumps as fuel for star formation. I matched 3,674 clumps from my catalog to 473 clouds from the COHRS catalog, a
590 ▼a School code: 0051.
650 4 ▼a Astrophysics.
650 4 ▼a Physics.
690 ▼a 0596
690 ▼a 0605
71020 ▼a University of Colorado at Boulder. ▼b Astrophysical and Planetary Sciences.
7730 ▼t Dissertation Abstracts International ▼g 80-02B(E).
773 ▼t Dissertation Abstract International
790 ▼a 0051
791 ▼a Ph.D.
792 ▼a 2018
793 ▼a English
85640 ▼u http://www.riss.kr/pdu/ddodLink.do?id=T14998165 ▼n KERIS ▼z 이 자료의 원문은 한국교육학술정보원에서 제공합니다.
980 ▼a 201812 ▼f 2019
990 ▼a ***1012033